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KMT-2024-BLG-3237: Another Free-floating Planet Candidate with Angular Einstein Radius Measurement

  • Authors: Tanagodchaporn Inyanya, Youn Kil Jung, Hongjing Yang, Kyu-Ha Hwang, Andrew Gould, Michael D. Albrow, Sun-Ju Chung, Cheongho Han, Yoon-Hyun Ryu, In-Gu Shin, Yossi Shvartzvald, Jennifer C. Yee, Weicheng Zang, Dong-Jin Kim, Chung-Uk Lee, Byeong-Gon Park

Tanagodchaporn Inyanya et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 3.

Gaia proper motions of stars in the vicinity (within ﹩6^{\prime} ﹩) of KMT-2024-BLG-3237. The red dots are red-giant (bulge-population) stars, while the blue dots are main-sequence (disk-population) stars. In each population, the inner and outer contours envelope 68% and 95% of the stars, respectively. The red square corresponds to the mean proper motion of the bulge population, 〈μbulge 〉 (lb) = (−6.22, −0.29) ± (3.28, 2.65) mas yr−1. The blue square is the mean proper motion of the disk population, 〈μdisk〉 (lb) = (−4.06, −0.74) ± (4.29, 3.06) mas yr−1. The baseline object (source) is located at the black dot. The black circle represents the locus of the relative lens-source proper motions, μrel = 4.29 mas yr−1.

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